- V1
LARGE CRYOGENIC GRAVITATIONAL-WAVE TELESCOPE
Drawing No
SPECIFICATION
Sheet 1
-D
Rev. Group
of
3
LCGT Power Recycling Mirror 3 (PR3)
AUTHOR:
Eiichi Hirose
CHECKED:
DATE
Nov21-11
DCN NO.
APPROVALS
REV
V1
DATE
Nov21-11
Applicable Documents
LCGT-MIR-D00006-V1 Fused Silica Substrate, LCGT PR3
LCGT-XXXXX-A
Fused Silica Blank, PR3
LCGT-XXXXX-A
Fused Silica Blank, PR3
Requirements
Physical Configuration
According to LCGT-MIR-D00006-V1 Fused Silica Substrate, LCGT PR3
Fabricate from
LCGT-XXXXX- A
LCGT-XXXXX- A
Fused Silica Blank, PR3
Fused Silica Blank, PR3
Registration Marks
Registration marks shall be etched, ground or sandblasted and located per LCGT-MIR-D00006-V1
Side and Bevel Polish
All surfaces, including Sides and Bevels shall be polished using a progression of smaller grit sizes. The last step before
final polish shall be equal to or less than a five micrometer grit finish. These surfaces shall appear transparent with no
grey, scuffs or scratches visible to the naked eye when viewed in normal room light against a black background.
Bevel
Bevel for safety per LCGT-MIR-D00006-V1
Serial Number
Serial Number “PR3 YY” shall be shall be etched, ground or sandblasted on the barrel of the optic per LCGTMIR-D00006-V1, where Y is incremental starting with 01.
Scratches, Sleeks and Point defects
Point defects of radius greater than 25 micrometers are treated like scratches for the purpose of this
specification.
LCGT MIR SPEC Form 01
- V1
LARGE CRYOGENIC GRAVITATIONAL-WAVE TELESCOPE
Drawing No
SPECIFICATION
Sheet 2
-D
Rev. Group
of
3
LCGT Power Recycling Mirror 3 (PR3)
Scratches and Sleeks, Surface 1
5
The total area of scratches and sleeks within the central 120 mm diameter shall not exceed 5 X 10 square
micrometers (width times length.)
Point Defects, Surface 1
There shall be no more than 50 point defects of radius greater than 2 m within the central 120 mm diameter.
Scratch and Point Defect Inspection Method
1. The surface is examined visually by two observers independently. The examination is done against a dark
background using a fiber optic illumination system of at least 200 W total power. A 100% inspection of the
surface is carried out. Pits and scratches down to 2 micrometers in width can be detected using this method of
inspection. Any scratches or sleeks that are detected will be measured using a calibrated eyepiece.
2. Further inspection will be done with a minimum 6X eyeglass using the same illumination conditions, again
with two observers. Sleeks down to 0.5 micrometers wide can be detected using this method. The surface will
be scanned along one or two chords from centre to edge, then at ten positions around the edge, and ten to fifteen
positions near the centre.
3. An inspection is then carried out with a dark or bright field microscope, with 5x objective at four positions at
each of the following locations:
a)
Within 5mm of the center of the surface.
b) Equally spaced along the circumference of a centered, 60 mm diameter circle.
c)
Equally spaced along the circumference of a centered, 120 mm diameter circle.
Optical Surface Figure, measured over the central 40 mm diameter
Surface 1: Spherical, concave. Radius of curvature: 24.57 m -0.10m, +0.10 m absolute accuracy
Astigmatism: < 30 nm Amplitude of the Zernike coefficient Z as defined in Born and Wolf pp. 523-525.
2, 2
Surface 2: Nominally flat. ROC > |7000m|
Surface Error, Low Spatial Frequency: measurement aperture to 1 mm-1
The following root mean square standard deviation (σ
rms
) values are calculated from the phase maps which are
to be provided with each optic. For this calculation the amplitudes for the best fit Zernike terms Z , Z , Z
0,0
and Z
2,2
1,1
2,0
or corresponding Seidel aberrations are subtracted from the phase map. Known bad pixels may be
excluded from this calculation.
-1
Surface 1, Frequency Band: < 1 mm
Measured outside the central 200 mm diameter aperture: σ
Measured over the central 150 mm diameter aperture: σ
rms
rms
< 3 nanometers
< 2 nanometers
-1
Surface 2, Frequency Band: < 1 mm
Measured outside the central 200 mm diameter aperture: σ
rms
< 40 nanometers
LCGT MIR SPEC Form 01
- V1
LARGE CRYOGENIC GRAVITATIONAL-WAVE TELESCOPE
Drawing No
SPECIFICATION
Sheet 3
-D
Rev. Group
of
3
LCGT Power Recycling Mirror 3 (PR3)
Error, High Spatial Frequency: 1– 750 mm
Surface 1 HSF error σ
rms
-1
< 0.3 nanometers
Measured at the following locations:
1. Within 2mm of the center of the surface.
2. Four positions equally spaced along the circumference of a centered, 10 mm diameter circle.
3. Three positions equally spaced along the circumference of a centered, 20 mm diameter circle.
Inspection
Table 1: Inspections
Specification
Dimensions
Test Method and
frequency
Measurement
100%
Data Delivered
Measurement Results
Scratches and Point defects
methods 1 and 2
Visual Inspection
100%
Hand sketch including scratch/pit
dimensions
Scratches and Point defects
method 3
Visual Inspection
100%
Digital image of each inspection location
Figure
Interferometry
100%
Interferometry
100%
Surface phase maps
Interferometry
100%
Surface maps for 3 central locations.
Numerical values included with
certification
Errors - Low Spatial Frequency
Errors - High Spatial Frequency
Surface phase maps
Orientation: For the purpose of full surface phase maps the data shall be oriented such that the substrate
registration mark is at the top center of the data.
Format: All Data shall be delivered according to Table 1. In addition to the hard copy, an electronic data set of
the phase maps shall be delivered in ASCII format.
LCGT MIR SPEC Form 01